Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-02T17:27:17.030295Z
Paper Citation Record · LEDGER
The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
As of 8 August 2026, this Paper Citation Record lists 2 of 2 outbound references and 7 inbound Pith citation observations for arXiv:2603.26200.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-02T16:51:29.879469Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Reference resolution
2 of 2 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved1
- parse uncertain0
- malformed identifier1
- metadata mismatch0
External citation measurements
0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
Observation 6a50eb9f-5373-4025-a149-fafcac42a99c · outbound
This paper cites 2022, Phys.
The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations 2022, Phys
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T17:27:17.025812Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2f0cc572-417e-464a-bf6f-b3a24e2fe195 · outbound
This paper cites arXiv:2510.17770 Huang K.-H., et al., 2017, ApJ, 838, 6 Hunter J.
The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations arXiv:2510.17770 Huang K.-H., et al., 2017, ApJ, 838, 6 Hunter J
Reference 1949
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-02T17:27:17.030295Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 97e32b6f-688c-4285-bd09-61bf30712568 · inbound
The morphologies of present-day galaxies in the COLIBRE simulations cites this paper.
The morphologies of present-day galaxies in the COLIBRE simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 82
- Resolution
- verified exact
- arxiv_id, observed 2026-07-29T01:24:31.270121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation f68422ca-fd3a-40df-aaf7-ee19a31f4ff0 · inbound
The morphologies of present-day galaxies in the COLIBRE simulations cites this paper.
The morphologies of present-day galaxies in the COLIBRE simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T16:51:29.879469Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8c249ada-5331-48a9-ae2b-e8b1322a2910 · inbound
Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations cites this paper.
Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 74
- Resolution
- verified exact
- arxiv_id, observed 2026-07-29T01:24:31.270121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation ca09d668-7f82-4b41-b323-5ff9de5fb3d9 · inbound
The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations cites this paper.
The galaxy ultraviolet luminosity function from $z=7$ to $15$ in the COLIBRE simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 119
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-29T01:24:31.270121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation d2494868-3008-414e-ad97-2d711bceeab8 · inbound
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations cites this paper.
The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 223
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-29T01:24:31.270121Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation b2e399e7-6808-442b-94e2-7e9b0a42f148 · inbound
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy cites this paper.
How large can galaxies be? Ultra-deep imaging of IC 1101, the most extended known galaxy The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T23:42:31.591767Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7d331190-99de-468d-a62b-10e033a1e5dd · inbound
The influence of feedback on the baryonic content of haloes in the COLIBRE simulations cites this paper.
The influence of feedback on the baryonic content of haloes in the COLIBRE simulations The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Reference 85
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T09:38:48.994603Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.